Abstract

We carry out numerical experiments in the critical collapse of a spherically symmetric massless scalar field in 2+1 spacetime dimensions in the presence of a negative cosmological constant and compare them against a new theoretical model. We approximate the true critical solution as the n=4n=4 Garfinkle solution, matched at the lightcone to a Vaidya-like solution, and corrected to leading order for the effect of Λ<0Λ<0. This approximation is only C3C^3 at the lightcone and has three growing modes. We {\em conjecture} that pointwise it is a good approximation to a yet unknown true critical solution that is analytic with only one growing mode (itself approximated by the top mode of our amended Garfinkle solution). With this conjecture, we predict a Ricci-scaling exponent of γ=8/7γ=8/7 and a mass-scaling exponent of δ=16/23δ=16/23, compatible with our numerical experiments.

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